Puppis
Puppis (/ˈpʌpɪs/) is a constellation in the southern sky. Puppis, the Latin translation of "poop deck", was originally part of an over-large constellation Argo Navis (the ship of Jason and the Argonauts), which centuries after its initial description, was divided into three parts, the other two being Carina (the keel and hull), and Vela (the sails of the ship). Puppis is the largest of the three constellations in square degrees. It is one of the 88 modern constellations recognized by the International Astronomical Union.
| Constellation | |
| Abbreviation | Pup |
|---|---|
| Genitive | Puppis |
| Pronunciation | /ˈpʌpɪs/, genitive the same |
| Symbolism | the Poop Deck |
| Right ascension | 7.5h |
| Declination | −30° |
| Quadrant | SQ2 |
| Area | 673 sq. deg. (20th) |
| Main stars | 9 |
| Bayer/Flamsteed stars | 76 |
| Stars with planets | 6 |
| Stars brighter than 3.00m | 1 |
| Stars within 10.00 pc (32.62 ly) | 3 |
| Brightest star | ζ Pup (Naos) (2.25m) |
| Messier objects | 3 |
| Meteor showers | Pi Puppids Zeta Puppids Puppid-Velids |
| Bordering constellations | Monoceros Pyxis Vela Carina Pictor Columba Canis Major Hydra |
| Visible at latitudes between +40° and −90°. Best visible at 21:00 (9 p.m.) during the month of February. | |
Features edit
Argo Navis was sub-divided into three sections in 1752 by the French astronomer Nicolas Louis de Lacaille, including Argûs in puppi. Despite the division, Lacaille kept a single set of Bayer designations for the whole constellation, Argo. Therefore, Carina has the α, β, and ε, Vela has γ and δ, Puppis has ζ, and so on.[1] In the 19th century, these three sections of Argo became established as separate constellations and were formally included in the list of 88 modern IAU constellations in 1930.[2]
Named stars edit
| Bayer designation | Name | Origin | Meaning |
|---|---|---|---|
| ζ | Naos | Greek | ship |
| ρ | Tureis | Arabic | shield |
| ξ | Asmidiske | Greek | gunwale |
Planetary systems edit
Several extrasolar planet systems have been found around stars in the constellation Puppis, including:
- On July 1, 2003, a planet was found orbiting the star HD 70642. This planetary system is much like Jupiter with a wide, circular orbit and a long-period.
- On May 17, 2006, HD 69830 (the nearest star of this constellation) was discovered to have three Neptune-mass planets, the first multi-planetary system without any Jupiter-like or Saturn-like planets. The star also hosts an asteroid belt at the region between middle planet to outer planet.
- On June 21, 2007, the first extrasolar planet found in the open cluster NGC 2423, was discovered around the red giant star NGC 2423-3. The planet is at least 10.6 times the mass of Jupiter and orbits at 2.1 AU distance.
- On September 22, 2008, two Jupiter-like planets were discovered around HD 60532. HD 60532 b has a minimum mass of 1.03 MJ and orbits at 0.759 AU and takes 201.3 days to complete the orbit. HD 60532 c has a minimum mass of 2.46 MJ and orbits at 1.58 AU and takes 604 days to complete the orbit.
- In 2023, Astronomers detected two ice giant type exoplanets (both with a mass of tens of earths) having a collision event around the 300 million year old star designated as 2MASS J08152329-3859234.
Deep-sky objects edit
As the Milky Way runs through Puppis, there are many open clusters in the constellation. M46 and M47 are two open clusters in the same binocular field. M47 can be seen with the naked eye under dark skies, and its brightest stars are 6th magnitude. Messier 93 (M93) is another open cluster somewhat to the south. NGC 2451 is a very bright open cluster containing the star c Puppis, and the near NGC 2477 is a good target for small telescopes. The star Pi Puppis is the main component of a bright group of stars known as Collinder 135.
M46 is a circular open cluster with an overall magnitude of 6.1 at a distance of approximately 5400 light-years from Earth. The planetary nebula NGC 2438 is superimposed; it is approximately 2900 light-years from Earth. M46 is classified as a Shapley class f and a Trumpler class III 2 m cluster. This means that it is a rich cluster that appears distinct from the star field. However, it is not at its center. The cluster's stars, numbering between 50 and 100, have a moderate range in brightness.[3]
See also edit
References edit
- ^ Wagman, M. (2003). Lost Stars: Lost, Missing, and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. McDonald & Woodward Publishing Company. ISBN 978-0-939923-78-6.
- ^ Delporte, E. (1930). Delimitation Scientifique des constellations (tables et cartes). Cambridge University Press. Bibcode:1930dsct.book.....D.
- ^ Levy 2005, pp. 85–86.
Sources edit
- Levy, David H. (2005), Deep Sky Objects, Prometheus Books, ISBN 1-59102-361-0
- Ian Ridpath and Wil Tirion (2017). Stars and Planets Guide, Collins, London. ISBN 978-0-00-823927-5. Princeton University Press, Princeton. ISBN 978-0-691-17788-5.
- Richard Hinckley Allen, Star Names, Their Lore and Legend, New York, Dover.
External links edit
- The Deep Photographic Guide to the Constellations: Puppis
- Star Tales – Puppis